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World's First Discovery of Physical Evidence Suggesting Large-Scale Mass Transfer in Solar System 4.5 Billion Years Ago - Clarification of origin of trans-Neptunian objects and a milestone for a new solar system formation model (Press Release)

Release Date
19 Sep, 2008
  • BL47XU (HAXPES / uCT)
Chondrules formed in the high-temperature region inside the solar system were successfully identified in an ultrafine substance emitted from a short-period comet (a trans-Neptunian object) in joint research by Kyushu University, Ibaraki University, Osaka University, University of Wisconsin, National Aeronautics and Space Administration (NASA), Japan Synchrotron Radiation Research Institute (JASRI), and Advanced Industrial Science and Technology (representative: Tomoki Nakamura, associate professor of Department of Earth and Planetary Science, Faculty of Science, Kyushu University). The chondrules were highly likely to have been transferred from the inside to the outside of early solar nebula because the oxygen isotope ratio of the chondrules discovered was similar to that of the chondrules in primitive objects in the asteroid belt of the solar system. It is difficult to fully explain this mass transfer with the current solar system formation model, and thus, a new model is required.

This achievement was published in Science on 19 September 2008 (Eastern US time).


(A) An electron microscope cross-sectional image of an ultrafine substance emitted from a short-period comet (a trans-Neptunian object).
(B) 11 holes show the spots at which the oxygen isotope ratios were measured.
(C) The oxygen isotope ratios measured. The data numbers correspond to those in (B).
(A) An electron microscope cross-sectional image of an ultrafine substance emitted from a short-period comet (a trans-Neptunian object).
(B) 11 holes show the spots at which the oxygen isotope ratios were measured.
(C) The oxygen isotope ratios measured. The data numbers correspond to those in (B).


For more information, please contact:
Dr. Tomoki Nakamura, Department of Earth and Planetary Science, Faculty of Science, Kyushu University)
e-mail:mail

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